TYC 3551-1177-1 , the SIMBAD biblio

TYC 3551-1177-1 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST02:36:55


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Title First 3 Authors
2014ApJS..210....1C viz 16       D               1 519 296 Asteroseismic fundamental properties of solar-type stars observed by the NASA Kepler mission. CHAPLIN W.J., BASU S., HUBER D., et al.
2015ApJ...808..187B viz 16       D               1 540 73 The metallicities of stars with and without transiting planets. BUCHHAVE L.A. and LATHAM D.W.
2016AJ....152....6W viz 16       D               1 3060 13 Calibration of LAMOST stellar surface gravities using the Kepler asteroseismic data. WANG L., WANG W., WU Y., et al.
2016A&A...594A..39F viz 16       D               2 51408 86 Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al.
2017ApJ...844..102H viz 16       D               1 2236 180 Asteroseismology and Gaia: testing scaling relations using 2200 Kepler stars with TGAS parallaxes. HUBER D., ZINN J., BOJSEN-HANSEN M., et al.
2018ApJ...858...28V viz 16       D               1 459 13 Investigating the metallicity-mixing-length relation. VIANI L.S., BASU S., ONG J.M.J., et al.
2018ApJ...861..149F viz 16       D               1 2261 6 The Kepler Follow-up Observation Program. II. Stellar parameters from medium- and high-resolution spectroscopy. FURLAN E., CIARDI D.R., COCHRAN W.D., et al.
2019ApJ...879...69T viz 17       D               1 222609 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., et al.
2020AJ....160..120J viz 17       D               1 365761 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2021AJ....161..170S viz 17       D               1 16187 ~ The Swan: data-driven inference of stellar surface gravities for cool stars from photometric light curves. SAYEED M., HUBER D., WHEELER A., et al.

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